The structure and spectra of irradiated secondaries in close binaries (pre-CVs)

Alexander Christopher Wawrzyn
Many stars evolve not alone but along one or more companions. While the evolution of single isolated stars is well predicted by theoretical calculations, close binary systems with their interactions are on the one hand far more difficult to handle, but on the other hand well constrained in their masses and sizes. One mechanism thought to produce such close binaries is the Common Envelope Evolution (CEE). Especially young post CEE binaries show great temperature differences...
This data repository is not currently reporting usage information. For information on how your repository can submit usage information, please see our documentation.